universe ka jo sabse strongest material nuclear pasta jo ke neutron star ke core me paya jata hai.
How much time nuclear pasta stronger than steel??
how dense it is ??
what is the properties of nuclear pasta???
nuclear pasta kese form hota hai . or neutron star me he kyu paya jata hai ?
kya or koi material hai es universe me jo nuclear pasta se bhe zyda strong hai ??
don't copy from Google..
I need exact answer.
only for true space lover.
jinko nehi aata wo yaha apna dimag na lagaye Google se chaap ke.
dhanyavaad.
Answers
Answer:
The physics at work inside a neutron star can be mind-bogglingly complex. The neutrons that are well-understood in the rest of the universe do strange things when exposed to such incredible pressure. A new analysis of this so-called “nuclear pasta” suggests matter inside a neutron star is the strongest material in the universe.
A neutron star is the dead husk of a star more massive than the sun, but not large enough to become a black hole upon its demise. These stars are between 10 and 29 solar masses during their active lifetime. When they exhaust their nuclear fuel and go supernova, all that’s left is the ultra-dense collapsed core. We call that a neutron star.
The wild physics inside a neutron star are down to the incredible mass packed into such a small space. A neutron star might have twice the mass of our sun packed into an object just a few miles across. The crush of gravity contorts and squeezes neutrons into unusual configurations, based on the models developed by scientists studying neutron stars.
Scientists currently believe that neutron stars have layers characterized by different configurations of distorted neutron matter. For whatever reason, researchers have decided to name the various structures after pasta. Near the surface there’s gnocchi, which are round bubble-like neutrons. Go a bit deeper, and the pressure forces neutrons into long tubes called spaghetti. Go further down, and you have sheets of neutrons called lasagna. That’s just the start of the Italian-inspired interior of neutron stars.
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